Grains orbiting a star experience orbital decay due to Poynting-Robertson drag and can become trapped in commensurability resonances with a planet. We examine conditions for trapping in the circular restricted three-body problem, and derive criteria for trapping in terms of the radiation pressure fa
β¦ LIBER β¦
Poynting-Robertson drag and orbital resonance
β Scribed by R. Gonczi; Ch. Froeschle; Cl. Froeschle
- Publisher
- Elsevier Science
- Year
- 1982
- Tongue
- English
- Weight
- 880 KB
- Volume
- 51
- Category
- Article
- ISSN
- 0019-1035
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